Upper panel: peak flux values (dots) and 3σ upper limits (triangles) of the JVLA observations in L- and C-bands (black and orange data points), and GMRT in band 4 (red data points), as a function of the observing epoch. Middle panel: ASAS-SN ɡ-band magnitudes and JVLA radio fluxes phase-folded to the stellar rotation period P~2.9 days. Phase zero corresponds to the first epoch of the JVLA C-band observations. Optical and radio observations were carried out within the same time span. Lower panel: GLS periodogram of the ASAS-SN optical light curve collected over the time span covered by JVLA observations (28 July–28 Sept. 2024). The stellar rotation period of ~2.9 days is indicated by a red dashed line.